A dataset provided by the European Space Agency

Name: Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys II
Published: 2018-03-29T22:00:00Z

Proposal ID	078120
Title	Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys II
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781200401
DOI	https://doi.org/10.5270/esa-69c05ka
Principal Investigator, PI	Prof Nobuhiro Okabe
Abstract	In continuation of our AO15-approved proposal, we hereby propose to completeXMM- Newton observations for a systematic study to calibrate cluster observablescaling relations, using precision, HSC-derived, weak lensing mass measurementsand make a stringent test of the assumption of hydrostatic equilibrium ofclusters. The exquisite quality of multi-band HSC imaging will enable us toimprove both the precision and accuracy of weak-lensing mass measurements. Bycombining these weak lensing mass measurements with deep X-ray and ACTPolSunyaev-Zel dovich effect data, we will have an unprecedented ability toconstrain the physical state of the ICM. Our project provides an essentialbridge to future, cluster-based, cosmological studies by eROSITA.
Publications	Multiwavelength study of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field \|Miyaoka Keita Okabe Nobuhiro et al. \| PASJ \| 70-22 \| 2018 \| 2018PASJ...70S..22M \| http://ui.adsabs.harvard.edu/#abs/2018PASJ...70S..22M ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters \|Tarrio P. Melin J.-B. \| A&A \| 626-7 \| 2019 \| 2019A&A...626A...7T \| http://ui.adsabs.harvard.edu/#abs/2019A&A...626A...7T The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava S. Giles P. A. et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Scaling relations of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Poon Helen Okabe Nobuhiro et al. \| MNRAS \| 520-6001 \| 2023 \| 2023MNRAS.520.6001P \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.520.6001P The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P Nature of the diffuse emission sources in the H I supershell in the galaxy IC 1613 \|Yarovova Anastasiya D. Moiseev Alexei V. et al. \| MNRAS \| 529-4930 \| 2024 \| 2024MNRAS.529.4930Y \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.4930Y From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-06-26T01:47:31Z/2017-01-21T03:40:11Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2018-03-29T22:00:00Z
Last Update	2025-01-27
Keywords	"stringent test", "exquisite quality", "ao15 approved", "actpol surveys ii", "complete xmm newton", "XMM", "deep xray", "hydrostatic equilibrium"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Nobuhiro Okabe, 2018, 'Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys II', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-69c05ka